WP3: Stellar winds and dust formation

Main contributors:
Bernhard Aringer, Sara Bladh

The purpose of WP3 is to supply grids of hydrostatic atmospheres and dynamical models including pulsation and dust-driven winds in order to compute spectra and photometric properties usable for WP4 and WP5, and mass-loss rates usable for WP1 as a function of stellar parameters.